Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
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p-process
Available isotopes for Sulfur (Z=16)
  32S   33S   34S   35S   36S
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Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
32S 33S




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
1.05.67 ± 0.83--
0.04.1 ± 0.6--

(Version 0.0 corresponds to Bao et al.)
Comment
Rec. value is from recent evaluations (endfb71,jendl40) assuming 15 % uncertainty.
Last review: February, 2013
List of all available values
originalrenorm.yeartypeCommentRef
4.1 ± 0.6
1980rLinac, TOF, 6Li, Au:Sat. Recalcul. including data of MDH81HJW80
4.2 ± 0.2
1980cLinac, TOF, 6Li ;Au:Sat.HJW80
5.84
2014eJEFF-3.2jeff32
5.67
2011eENDF/B-VII.1endfb71
5.67
2011eJENDL-4.0jendl40
5.67
2004eJEFF-3.1jeff31
3.0 ± 0.6
1971eAGM71
25.9
2005tMOST 2005Gor05
43.1
2002tMOST 2002Gor02
11.15
2000tNON-SMOKERRaT99
4.9
1978tWFH78


Original:MACS [<σ v>/vT] (mb) for kT=30 keV, based on the published cross sections except where indicated otherwise.
Renorm:MACS [<σ v>/vT] (mb) for kT=30 keV for which the reference or standard cross section was meanwhile improved.
Type: The letters and numbers in the column labelled 'type' give information on how the cross section has been obtained:
rRecalculated for kT = 30keV with the code described in Ref. 2 after renormalizing the original data to updated standard cross sections
cDirectly quoted from the reference itself
eEvaluated value taken directly from the reference
tTheoretical value
MACS, SEF and Reaction Rates for different energies
Energy5keV8keV10keV15keV20keV25keV30keV40keV50keV60keV80keV100keV
MACS
1.31
-
3.84
5.23
5.68
5.76
5.67 ± 0.83
5.29
4.85
4.44
3.77
3.28
Xfactor1.001.001.001.001.001.001.001.001.001.001.001.00
SEF1.001.001.001.001.001.001.001.001.001.001.001.00
Rate
7.87
-
32.61
54.40
68.22
77.34
83.40
89.85
92.10
92.36
90.55
88.08

MACS:
Reference: endfb71,jendl40
Procedure: 'e+t' (The MACS from kT=5 keV to 100 keV are derived from calculated cross sections, which are then normalized to experimental data, e.g. to the values at kT=25 keV obtained in activation measurements. In these cases the uncertainties should be linearly increased below 25 and above 30 keV to reach about 30% at the extreme kT values.)
Year: 2011

X-factor:
Reference: Rau12
Year: 2012

SEF (Stellar enhancement factor):
Reference: Rau09
Year: 2009
Comment:

Rate:
Reaction rate NA<σv> given in 104 cm3/mole/s, including SEF
Chart of nuclei
up
left
32Ar
98.00 ms
β+
33Ar
173.00 ms
β+
34Ar
845.00 ms
β+
35Ar
1.77 s
β+
36Ar
0.3365
9 mb
31Cl
150.00 ms
β+
32Cl
298.00 ms
β+
33Cl
2.51 s
β+
34Cl
1.53 s
β+
35Cl
75.77
10 mb
30S
1.18 s
β+
31S
2.57 s
β+
32S
95.02
4.1 mb
33S
0.75
7.4 mb
34S
4.21
0.226 mb
29P
4.14 s
β+
30P
2.50 m
β+
31P
100
1.74 mb
32P
14.26 d
β-
33P
25.34 d
β-
28Si
92.23
2.9 mb
29Si
4.683
7.9 mb
30Si
3.087
6.5 mb
31Si
2.62 h
β-
32Si
132.02 a
β-
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Isotope: Sulfur